Abstract
In these lecture notes we will give a very basic introduction to supermassive black holes. We derive the basic luminosity expected for accretion and introduce the Eddington limit. Kinematical evidence for black holes in the centers of galaxies from optical and radio spectroscopy is discussed as well as the link between black holes and host galaxy properties. Finally we consider the evidence for the black hole in the Galactic Center.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.